Massive compact dwarf stars and C-field
Astrophysics
2009-10-28 v1
Abstract
The effect of C-field in high density matter has been studied. We find that the negative energy and negative pressure of the C-field helps in formation of massive compact stable neutron stars of mass 0.5 solar mass which is in the range of 0.01 to 1.0 solar mass of recently observed dwarf stars.
Keywords
Cite
@article{arxiv.astro-ph/9601075,
title = {Massive compact dwarf stars and C-field},
author = {L. P. Singh and P. K. Sahu},
journal= {arXiv preprint arXiv:astro-ph/9601075},
year = {2009}
}
Comments
10 pages (LaTex), one figure available upon request